MHD numerical simulations of colliding winds in massive binary systems: I. Thermal versus non-thermal radio emission (2012)
- Authors:
- USP affiliated authors: ABRAHAM, ZULEMA - IAG ; GONÇALVES, DIEGO ANTONIO FALCETA - EACH
- Unidades: IAG; EACH
- DOI: 10.1111/j.1365-2966.2012.20978.x
- Subjects: ESTRELAS; ESTRELAS BINÁRIAS; VENTO
- Language: Inglês
- Imprenta:
- Source:
- Título: Monthly Notices of the Royal Astronomical Society
- ISSN: 0035-8711
- Volume/Número/Paginação/Ano: v. 423, p. 1562-1570, 2012
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: bronze
-
ABNT
FALCETA-GONÇALVES, D e ABRAHAM, Zulema. MHD numerical simulations of colliding winds in massive binary systems: I. Thermal versus non-thermal radio emission. Monthly Notices of the Royal Astronomical Society, v. 423, p. 1562-1570, 2012Tradução . . Disponível em: https://doi.org/10.1111/j.1365-2966.2012.20978.x. Acesso em: 05 nov. 2024. -
APA
Falceta-Gonçalves, D., & Abraham, Z. (2012). MHD numerical simulations of colliding winds in massive binary systems: I. Thermal versus non-thermal radio emission. Monthly Notices of the Royal Astronomical Society, 423, 1562-1570. doi:10.1111/j.1365-2966.2012.20978.x -
NLM
Falceta-Gonçalves D, Abraham Z. MHD numerical simulations of colliding winds in massive binary systems: I. Thermal versus non-thermal radio emission [Internet]. Monthly Notices of the Royal Astronomical Society. 2012 ; 423 1562-1570.[citado 2024 nov. 05 ] Available from: https://doi.org/10.1111/j.1365-2966.2012.20978.x -
Vancouver
Falceta-Gonçalves D, Abraham Z. MHD numerical simulations of colliding winds in massive binary systems: I. Thermal versus non-thermal radio emission [Internet]. Monthly Notices of the Royal Astronomical Society. 2012 ; 423 1562-1570.[citado 2024 nov. 05 ] Available from: https://doi.org/10.1111/j.1365-2966.2012.20978.x - The Bardeen-Petterson effect as the precession mechanism for the radio galaxy 3C 84 (NGC 1275)
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Informações sobre o DOI: 10.1111/j.1365-2966.2012.20978.x (Fonte: oaDOI API)
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